Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jmosp.153..718d&link_type=abstract
Journal of Molecular Spectroscopy, Volume 153, Issue 1-2, p. 718-725.
Astronomy and Astrophysics
Astrophysics
36
Scientific paper
Band origins and Einstein A coefficients are presented for transitions linking all the vibrational levels of H3+ up to 4ν2(l = 4). The importance of these data for astrophysical modeling is discussed. For H3+, rovibrational wavefunctions and energy levels are obtained for J up to 16. These are used to synthesize sample rovibrational spectra with particular emphasis on the ν1 + 2ν2(l = 2) <-- 0 and 4ν2(l = 2) <-- 0 bands, which would appear to be good candidates for laboratory observation.
Dinelli Bianca M.
Miller Steven
Tennyson Jonathan
No associations
LandOfFree
Bands of H3+ up to 4ν2: Rovibrational transitions from first principles calculations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Bands of H3+ up to 4ν2: Rovibrational transitions from first principles calculations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bands of H3+ up to 4ν2: Rovibrational transitions from first principles calculations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1518524